The main science is performed by Integral Field Spectrograph (IFS) CHARIS using J-, H-, and K-band (1.1 to 2.4 µm). CHARIS has a field of view 2 by 2 arcsecond with two different modes. The low-resolution mode (R\(\approx \) 20) uses broadband light between J- and K-bands while the high-resolution mode (R\(\approx \) 70) performs single band spectroscopy at J-, H-, or K-band. Using CHARIS typically observes exoplanets, protoplanetary and debris disks and performs spectral characterization[1]}, [2]}, [3]}, [4]}, [5]}, [6]}, [7]}, [8]}.
